Iinkcukacha
| RM-CPHA1015-20 | ||
| Iiparamitha | Inkcazo | Iyunithi |
| Uluhlu lokuphindaphinda | 10-15 | GHz |
| Inzuzo | 20 Chwetheza. | dBi |
| VSWR | 1.2Chwetheza. |
|
| Ipolarization | I-LHCP |
|
| AR | <1.6 |
|
| I-Cross Polarization | 30 Isimbo. | dB |
| 3dB Beamwidth | 12-18 | deg |
| Ujongano | I-SMA-Ibhinqa |
|
| Izinto eziphathekayo | Al |
|
| Ukugqiba | Phayi |
|
| Amandla aphakathi | 50 | W |
| Amandla aphezulu | 100 | W |
| Ubungakanani(L*W*H) | 464.9*111.6*117.5 (±5) | mm |
| Ubunzima | 0.758 | kg |
I-Antenna yeSetyhula yePolarization Horn yi-eriyali yemicrowave ekhethekileyo eguqula imiqondiso yomgca elungelelanisiweyo ibe ngamaza ajikelezayo asasaziweyo ngokusebenzisa i-polarizer edibeneyo. Esi sixhobo sikhethekileyo senza ukuba sibaluleke ngakumbi kwizicelo apho uzinzo lwe-polarization yomqondiso lubalulekile.
Iimpawu eziphambili zobuGcisa:
-
ISetyhula yePolarization Generation: Isebenzisa i-dielectric okanye i-polarizer yentsimbi ukwenza imiqondiso ye-RHCP/LHCP
-
I-Low Axial Ratio: Ngokuqhelekileyo <3 dB, iqinisekisa ukucoceka okuphezulu kwe-polarization
-
I-Broadband Operation: Ngokubanzi ibandakanya i-1.5: i-1 frequency ratio bandwidths
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Iziko leSigaba esiZinzile: Ligcina iimpawu ezingaguqukiyo zemitha kwibhendi yamaza
-
Ukwahlukaniswa okuphezulu: Phakathi kwamacandelo e-orthogonal polarization (>20 dB)
Usetyenziso Olungundoqo:
-
Iinkqubo zonxibelelwano ngesathelayithi (ukoyisa iFaraday rotation effect)
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I-GPS kunye nabamkeli bokuhamba
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Iinkqubo zeRadar zemozulu kunye nezicelo zomkhosi
-
I-astronomy kanomathotholo kunye nophando lwenzululwazi
-
I-UAV kunye namakhonkco onxibelelwano ngeselula
Ukukwazi kwe-eriyali ukugcina imfezeko yomqondiso nokuba luluphi na utshintsho lokuqhelaniswa phakathi komthumeli kunye nomamkeli kuyenza ibaluleke kakhulu kunxibelelwano lwesathelayithi kunye nolweselfowuni, apho ukungafani komqondiso wepolarization kunokubangela ukuthotywa okukhulu.
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